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XMM-Newton explores the fossil galaxy cluster RX J1416.4+2315

Image

Minimum credit line: Image courtesy of Habib Khosroshahi (University of Birmingham) and ESA. (for details, see Conditions of Use).
Credit: ESA/XMM-Newton, CC BY-SA 3.0 IGO

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About this Image

The image shows an X-ray emitting cloud (blue) observed by XMM-Newton in the fossil galaxy cluster RX J1416.4+2315 together with an optical R-band image of the central galaxy. The cloud is three million light years across and temperatures inside it reach 50 million degrees. This cloud is believed to surround a giant elliptical galaxy which has formed from merging smaller galaxies. Dark matter in a group of galaxies holds the group together by gravitational attraction. This may cause larger galaxies to move towards the centre of the group and merge together into one giant galaxy. In a fossil group all of the galaxies have merged into one giant galaxy, surrounded by a dark matter halo. The dark matter halo gravitationally attracts hot gas, visible in X-ray emission as in this image.

Investigator(s):  H. Khosroshahi, B. Maughan, T. Ponman, L. Jones

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